SUMMARY OF PROPOSAL 41081
MR. ICHIZO HAYASHI
KYOTO UNIVERSITY
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWAOIWAKE-CHO SAKYO-KU

  E-mail: HAYASHI@CR.SCPHYS.KYOTO-U.AC.JP	Tel: +81-75-753-3851	Fax: +81-75-701-5377
  Medium: 2.5GB8MM

Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION            
  Title: ASCA SPECTROSCOPY OF AN OLD SNR IN THE SMC                                      


Abstract:
 SNR 0103-72.6 is the only "old SNR" in the Small Magellanic Cloud that has enough
 X-ray brightness for detaied spectral studies with ASCA. This SNR allows us to
 understand the relation between the SNR evolution and a wind blown bubble (DEM 125),
 and the connection between the SNR evolution and the host galaxy. It also provides
 us with reliable data for the SMC chemical abundances and the clues to solve the
 complex spectrum of the "young SNR" 0102-72.3 observed in the PV phase.

 Co-Is:
   1  KATSUJI KOYAMA      	KYOTO UNIVERSITY              JAPAN     
      (No Co-I contact data)
   2  IKUKO ASAOKA        	MAX PLANCK INSTITUTE          GERMANY   


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
0103-72.6              1   16.2167  -72.3864    80   N   Y   P  0.09000   1 

REMARKS:           THE SOURCE EXTENDS ABOUT 2 ARCMIN IN DIAMETER.